姿态抖动运动单平台LBI无源定位系统的角变化率估计和定位算法研究

 研究了采用长基线干涉仪(LBI)体制的运动单平台无源定位系统受平台姿态抖动影响的问题,指出由于平台姿态的快速无规则变化,相位差变化率(RPDC)方法将难以适用,应当采用目标方位角变化率参数进行定位。基于此,针对三维几何空间,提出了一种RP-LS方法估计目标方位角变化率,继而实现对目标的定位。仿真结果表明,该方法能有效解决LBI体制运动单平台定位系统对姿态抖动的适应问题,实现对目标的快速高精度定位。     

阻力伞附加质量与阻力系数修正方法

在阻力伞试验,特别是高速滑车试验过程中,由于阻力伞系统作非匀加速的非定常运动以及前置体尾流场的影响,现有的阻力伞试验数据计算方法已经难以准确计算其阻力系数.本文针对阻力伞试验过程中的这种非定常运动和尾流干扰特性,对阻力伞系统进行了动力学分析,并对阻力伞非定常运动过程中的附加质量和尾流场特性进行了理论研究,提出了阻力伞双...     

Space storm measurements of the July 2005 solar extreme events from the low corona to the Earth

The Athens Neutron Monitor Data Processing (ANMODAP) Center recorded an unusual Forbush decrease with a sharp enhancement of cosmic ray intensity right after the main phase of the Forbush decrease on 16 July 2005, followed by a second decrease within less than 12 h. This exceptional event is neither a ground level enhancement nor a geomagnetic effect in cosmic rays. It rather appears as the effect of a special structure of interplanetary disturbances originating from a group of coronal mass ejections (CMEs) in the 13–14 July 2005 period. The initiation of the CMEs was accompanied by type IV radio bursts and intense solar flares (SFs) on the west solar limb (AR 786); this group of energetic phenomena appears under the label of Solar Extreme Events of July 2005. We study the characteristics of these events using combined data from Earth (the ARTEMIS IV radioheliograph, the Athens Neutron Monitor (ANMODAP)), space (WIND/WAVES) and data archives. We propose an interpretation of the unusual Forbush profile in terms of a magnetic structure and a succession of interplanetary shocks interacting with the magnetosphere.     

Modelling and observations of photospheric magnetic helicity

Mounting observational evidence of the emergence of twisted magnetic flux tubes through the photosphere have now been published. Such flux tubes, formed by the solar dynamo and transported through the convection zone, eventually reach the solar atmosphere. Their accumulation in the solar corona leads to flares and coronal mass ejections. Since reconnections occur during the evolution of the flux tubes, the concepts of twist and magnetic stress become inappropriate. Magnetic helicity, as a well preserved quantity, in particular in plasma with high magnetic Reynolds number, is a more suitable physical quantity to use, even if reconnection is involved.     

小型磁偏转质谱计性能实验研究

自主研发了小型磁偏转质谱计,并对其质量范围、分辨本领、灵敏度和最小可检分压力四个主要性能指标进行了实验测试和比对。结果表明,该质谱计的质量范围为（1~143）amu,相对N₂的分辨本领为1400,灵敏度为4.2×10^-5 A/Pa,最小可检分压力为9.5×10^-7 Pa。该测试和比对结果为磁偏转质谱计进一步的优化设计和性能提高奠定了重要基础。     

基于相位变化率的无源定位法

无源定位技术有着广阔的应用前景，本文在现有单站无源定位方法的基础上，介绍了相位变化率定位法。该方法利用观测平台上两个相互正交的相位干涉仪接收目标辐射电磁波的相位获取目标的方向信息，利用对应的相位变化率获取目标的径向距离信息，从而实现对目标的实时高精度定位。文中还给出了观测平台飞行姿态变化情况下的定位表达式。仿真结果表明，该方法是一种发展前途较好的单站无源定位方法。     

Geoeffectivity of Coronal Mass Ejections

Coronal mass ejections and post-shock streams driven by them are the most efficient drivers of strong magnetospheric activity, magnetic storms. For this reason there is considerable interest in trying to make reliable forecasts for the effects of CMEs as much in advance as possible. To succeed this requires understanding of all aspects related to CMEs, starting from their emergence on the Sun to their propagation to the vicinity of the Earth and to effects within the magnetosphere. In this article we discuss some recent results on the geoeffectivity of different types of CME/shock structures. A particularly intriguing observation is that smoothly rotating magnetic fields within CMEs are most efficient in driving storm activity seen in the inner magnetosphere due to enhanced ring current, whereas the sheath regions between the shock and the ejecta tend to favour high-latitude activity.     

星用非金属材料出气模型的应用

卫星上所用非金属材料，在空间真空环境下存在出气行为，产生污染效应。为了研究这种出气行为，本文以扩散理论为理论依据，推导材料出气模型。利用空间分子污染气体分析仪，测试了星用非金属材料的出气速率变化，对所测数据进行曲线拟合，通过试验和理论分析，证实了模型推导的正确性，结果表明：经过6h的真空加热预处理能够有效减少出气污染。     

原子氧对Kapton／Al薄膜性能影响研究

模拟空间环境下原子氧辐照条件,通过采用固定的原子氧束流密度进行不同时间辐照试验,研究了温控涂层材料Kapton/Al薄膜的质量损失、光学性能、表面形貌和表面粗糙度的演化规律.试验结果表明,原子氧对材料的剥蚀量与原子氧的作用时间成正比例关系.材料辐照后太阳吸收率发生明显变化,而辐射率几乎不发生变化.辐照后试样表面的粗糙度,是影响太阳吸收率变化主要因素.随着辐照时间的增长,材料表面粗糙度增加,导致太阳吸收率增大.     

发动机质心测试系统软硬件设计

介绍了发动机质心测试系统的基本构成以及其软硬件的设计实现.